Formation of chondrule fine‐grained rims from local nebular reservoirs-Reference-Cited by-同舟云学术

Formation of chondrule fine‐grained rims from local nebular reservoirs

Published:2022-03-31 Issue:5 Volume:57 Page:1004-1017
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit & Planetary Scien

Author:

Pinto Gabriel A.¹²^ORCID,Marrocchi Yves²^ORCID,Jacquet Emmanuel³^ORCID,Olivares Felipe¹^ORCID

Affiliation:

1. Instituto de Astronomía y Ciencias Planetarias Universidad de Atacama Copayapu 485 Copiapó Chile

2. Université de Lorraine CNRS CRPG UMR 7358 Vandœuvre‐lès‐Nancy 54501 France

3. Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie (IMPMC) Muséum national d'Histoire naturelle Sorbonne Université CNRS CP52, 57 rue Cuvier Paris 75005 France

Funder

Fondo Nacional de Desarrollo Científico y Tecnológico

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13812

Reference78 articles.

1. The Formation Conditions of Chondrules and Chondrites

2. Origin, age, and composition of meteorites

3. Bigolski J. N.2017.The Formation of Fine‐Grained Chondrule Rims in Unequilibrated Ordinary Chondrites. PhD thesis The City University of New York New York USA.

4. Microchondrules in three unequilibrated ordinary chondrites

5. Bigolski J. Weisberg M. K. Ebel D. S. andConnolly H. C.2014.Microchondrules: Records of Multiple Heating Events in the Solar Nebula and Implications for Type II Chondrule Formation (Abstract #1879). 45th Lunar and Planetary Science Conference. CD‐ROM.

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